A conspicuous clay ovoid in Nakhla: evidence for subsurface hydrothermal alteration on Mars with implications for astrobiology.
A conspicuous clay ovoid in Nakhla: evidence for subsurface hydrothermal alteration on Mars with implications for astrobiology.
复制标题
纳赫拉的一个明显的粘土卵形体:火星地下热液蚀变的证据对天体生物学的影响。
DOI:
10.1089/ast.2013.1069
复制
发表时间:
2014
期刊:
影响因子:
4.2
通讯作者:
Chatzitheodoridis E
中科院分区:
文献类型:
--
作者:
Chatzitheodoridis E
A conspicuous biomorphic ovoid structure has been discovered in the Nakhla martian meteorite, made of nanocrystalline iron-rich saponitic clay and amorphous material. The ovoid is indigenous to Nakhla and occurs within a late-formed amorphous mesostasis region of rhyolitic composition that is interstitial to two clinopyroxene grains with Al-rich rims, and contains acicular apatite crystals, olivine, sulfides, Ti-rich magnetite, and a new mineral of the rhoenite group. To infer the origin of the ovoid, a large set of analytical tools was employed, including scanning electron microscopy and backscattered electron imaging, wavelength-dispersive X-ray analysis, X-ray mapping, Raman spectroscopy, time-of-flight secondary ion mass spectrometry analysis, high-resolution transmission electron microscope imaging, and atomic force microscope topographic mapping. The concentric wall of the ovoid surrounds an originally hollow volume and exhibits internal layering of contrasting nanotextures but uniform chemical composition, and likely inherited its overall shape from a preexisting vesicle in the mesostasis glass. A final fibrous layer of Fe-rich phases blankets the interior surfaces of the ovoid wall structure. There is evidence that the parent rock of Nakhla has undergone a shock event from a nearby bolide impact that melted the rims of pyroxene and the interstitial matter and initiated an igneous hydrothermal system of rapidly cooling fluids, which were progressively mixed with fluids from the melted permafrost. Sharp temperature gradients were responsible for the crystallization of Al-rich clinopyroxene rims, rhoenite, acicular apatites, and the quenching of the mesostasis glass and the vesicle. During the formation of the ovoid structure, episodic fluid infiltration events resulted in the precipitation of saponite rinds around the vesicle walls, altered pyrrhotite to marcasite, and then isolated the ovoid wall structure from the rest of the system by depositing a layer of iron oxides/hydroxides. Carbonates, halite, and sulfates were deposited last within interstitial spaces and along fractures. Among three plausible competing hypotheses here, this particular abiotic scenario is considered to be the most reasonable explanation for the formation of the ovoid structure in Nakhla, and although compelling evidence for a biotic origin is lacking, it is evident that the martian subsurface contains niche environments where life could develop. Key Words: Biomorph—Clays—Search for life (biosignatures)—Martian meteorites—Hydrothermal systems. Astrobiology 14, 651–693.
登录
查看更多内容
影响因子:
2.3
作者:
Herrera, Aude;Cockell, Charles S.;Tindle, Andrew G.
通讯作者:
Tindle, Andrew G.
影响因子:
3.7
作者:
Li X;Bai L;Fang J;Hou S;Zhou Q;Yu H;Kijlstra A;Yang P
通讯作者:
Yang P
影响因子:
3.7
作者:
N. Stroncik;H. Schmincke
通讯作者:
N. Stroncik;H. Schmincke
影响因子:
4.2
作者:
D. Pullan;F. Westall;B. Hofmann;J. Parnell;C. Cockell;H. Edwards;S. Villar;C. Schröder;G. Cressey;L. Marinangeli;L. Richter;G. Klingelhöfer
通讯作者:
G. Klingelhöfer
影响因子:
3.2
作者:
J. Bandfield;E. Amador;N. Thomas
通讯作者:
N. Thomas